Search Publications

Nuclear Activity in the Low-metallicity Dwarf Galaxy SDSS J0944-0038 : A Glimpse into the Primordial Universe
DOI: 10.3847/2041-8213/acb4e4 Bibcode: 2023ApJ...946L..38R

Nyland, Kristina; Canalizo, Gabriela; Satyapal, Shobita +11 more

Local low-metallicity dwarf galaxies are relics of the early universe and are thought to hold clues into the origins of supermassive black holes. While recent studies are uncovering a growing population of active galactic nuclei (AGNs) in dwarf galaxies, the vast majority reside in galaxies with solar or supersolar metallicities and stellar masses…

2023 The Astrophysical Journal
eHST 11
The intense production of silicates during the final AGB phases of intermediate mass stars
DOI: 10.1051/0004-6361/202245501 Bibcode: 2023A&A...670A..97M

Dell'Agli, F.; Ventura, P.; Fabrizio, M. +7 more

Context. The formation of silicates in circumstellar envelopes of stars evolving through the asymptotic giant branch (AGB) is still highly debated given the uncertainties affecting stellar evolution modelling, the description of the dust formation process, and the capability of silicate grains to accelerate stellar outflows via radiation pressure.…

2023 Astronomy and Astrophysics
Gaia ISO 11
Using the Gaia Excess Uncertainty as a Proxy for Stellar Variability and Age
DOI: 10.3847/1538-4357/ace044 Bibcode: 2023ApJ...953..127B

Barber, Madyson G.; Mann, Andrew W.

Stars are known to be more active when they are young, resulting in a strong correlation between age and photometric variability. The amplitude variation between stars of a given age is large, but the age-variability relation becomes strong over large groups of stars. We explore this relation using the excess photometric uncertainty in Gaia photom…

2023 The Astrophysical Journal
Gaia 11
Innovative technique for separating proton core, proton beam, and alpha particles in solar wind 3D velocity distribution functions
DOI: 10.1051/0004-6361/202243719 Bibcode: 2023A&A...669A.108D

Fedorov, A.; Livi, S.; Louarn, P. +10 more

Context. The identification of proton core, proton beam, and alpha particles in solar wind ion measurements is usually performed by applying specific fitting procedures to the particle energy spectra. In many cases, this turns out to be a challenging task due to the overlapping of the curves.
Aims: We propose an alternative approach based on …

2023 Astronomy and Astrophysics
SolarOrbiter 11
A rotating white dwarf shows different compositions on its opposite faces
DOI: 10.1038/s41586-023-06171-9 Bibcode: 2023Natur.620...61C

Kulkarni, S. R.; Vennes, Stéphane; Hermes, J. J. +35 more

White dwarfs, the extremely dense remnants left behind by most stars after their death, are characterized by a mass comparable to that of the Sun compressed into the size of an Earth-like planet. In the resulting strong gravity, heavy elements sink towards the centre and the upper layer of the atmosphere contains only the lightest element present,…

2023 Nature
Gaia 11
A multiwavelength study of multiple spectral component jets in AGN: testing the IC/CMB model for the large-scale-jet X-ray emission
DOI: 10.1093/mnras/stac3081 Bibcode: 2023MNRAS.518.3222B

Georganopoulos, Markos; Breiding, Peter; Meyer, Eileen T. +3 more

Over ~150 resolved, kpc-scale X-ray jets hosted by active galactic nuclei have been discovered with the Chandra X-ray Observatory. A significant fraction of these jets have an X-ray spectrum either too high in flux or too hard to be consistent with the high-energy extension of the radio-to-optical synchrotron spectrum, a subtype we identify as Mul…

2023 Monthly Notices of the Royal Astronomical Society
eHST 11
Slow Solar Wind Connection Science during Solar Orbiter's First Close Perihelion Passage
DOI: 10.3847/1538-4365/acd24b Bibcode: 2023ApJS..267...11Y

D'Amicis, Raffaella; Teriaca, Luca; Hirzberger, Johann +76 more

The Slow Solar Wind Connection Solar Orbiter Observing Plan (Slow Wind SOOP) was developed to utilize the extensive suite of remote-sensing and in situ instruments on board the ESA/NASA Solar Orbiter mission to answer significant outstanding questions regarding the origin and formation of the slow solar wind. The Slow Wind SOOP was designed to lin…

2023 The Astrophysical Journal Supplement Series
Hinode IRIS SolarOrbiter 11
Blue Large-Amplitude Pulsators and Other Short-Period Variable Stars in the OGLE-IV Galactic Disk Fields
DOI: 10.32023/0001-5237/73.1.1 Bibcode: 2023AcA....73....1B

Soszyński, I.; Udalski, A.; Szymański, M. K. +12 more

Blue Large-Amplitude Pulsators (BLAPs) form a mysterious class of variable stars with typical periods of tens of minutes and amplitudes above 0.1 mag. In this work, we present results of a variability search focused on timescales shorter than 1 h, conducted in OGLE-IV Galactic disk fields containing about 1.1 billion stellar sources down to I≈20 m…

2023 Acta Astronomica
Gaia 11
UOCS-IX. AstroSat/UVIT Study of the Open Cluster NGC 2818: Blue Stragglers, Yellow Stragglers, Planetary Nebula, and their Membership
DOI: 10.3847/1538-4357/acb0c8 Bibcode: 2023ApJ...945...11R

Rao, N. Kameswara; Subramaniam, Annapurni; Rani, Sharmila +1 more

We present the first far-UV (FUV) imaging results of the intermediate-age Galactic open cluster NGC 2818 that has a planetary nebula (PN) within the field using images taken from the Ultra Violet Imaging Telescope (UVIT) aboard AstroSat. We identify cluster members by combining UVIT-detected sources with Gaia EDR3 data. We detect four bright and h…

2023 The Astrophysical Journal
Gaia 11
A search for transit timing variations within the exomoon corridor using Kepler data
DOI: 10.1093/mnras/stac3360 Bibcode: 2023MNRAS.518.3482K

Kipping, David; Yahalomi, Daniel A.

An exomoon will produce transit timing variations (TTVs) upon the parent planet and their undersampled nature causes half of such TTVs to manifest within a frequency range of two to four cycles, irrespective of exomoon demographics. Here, we search through published Kepler TTV data for such signals, applying a battery of significance and robustnes…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 11